The JUICE spacecraft is taking shape and the magnetometer boom is being tested in an innovative way.
ESA: A test version of the 10.5-m long magnetometer boom built for ESA’s mission to Jupiter, developed by SENER in Spain, seen being tested at ESA’s Test Centre in the Netherlands, its weight borne by balloons.
The flight model will be mounted on the Juice spacecraft – Jupiter Icy Moons Explorer – due to launch in 2022, arriving at Jupiter in 2029. The mission will spend at least three years making detailed observations of the giant gaseous planet Jupiter and three of its largest moons: Ganymede, Callisto and Europa.
The Juice spacecraft will carry the most powerful remote sensing, geophysical, and in situ payload complement ever flown to the outer Solar System. Its payload consists of 10 state-of-the-art instruments.
This includes a magnetometer instrument that the boom will project clear of the main body of the spacecraft, allowing it to make measurements clear of any magnetic interference. Its goal is to measure Jupiter’s magnetic field, its interaction with the internal magnetic field of Ganymede, and to study subsurface oceans of the icy moons.
The deployment of this qualification model boom has been performed before and after simulated launch vibration on Test Centre shaker tables to ensure it will deploy correctly in space. Since the boom will deploy in weightlessness, three helium balloons were used to help bear its weight in terrestrial gravity.
CHEOPS or Characterising Exoplanet Satellite is steadily moving towards a launch date later this year. Currently the satellite is at Airbus Defence and Space Spain, Madrid and will eventually be shipped to Kourou, French Guiana for launch.
ESA — This photograph, taken a short hike from the Geographic South Pole in Antarctica, shows some of the antennas comprising the Super Dual Auroral Radar Network (SuperDARN) array. They are visible here as the chain of antennas and wiring stretching away into the distance. The red lights along the horizon in the background are lights marking the entrances to the Amundsen-Scott research station, which lies a good kilometre distant.SuperDARN is a network of radar antennas that monitors and explores the geomagnetic effects occurring in the Earth’s upper atmosphere. While some of these antennas are located at the South Pole, the network stretches worldwide and antennas are found in both the northern and southern hemispheres. One such geomagnetic effect is neatly captured here as wispy curtains and streaks of green filling the dark night sky above the antennas themselves: an aurora.Auroras, informally known as polar lights, form as charged particles from the Sun flow into our region of space, hit the outer boundary of Earth’s magnetic field, and move further inwards to collide with the atoms and molecules in our planet’s atmosphere. The aurora seen here is known as aurora australis, or the southern lights.Such phenomena form a key component of ‘space weather’, dynamic changes in the Earth’s cosmic environment that are driven by the activity of the Sun. As these can affect the function of both space-borne and ground-based systems and services, it’s crucial to monitor space weather in order to predict and mitigate its adverse effects. ESA does so via the Space Situational Awareness Space Weather Segment, and various science missions such as Cluster and Swarm, along with dedicated Sun-watching satellites to better understand our nearest star as a complete system.This image was taken by ESA research fellow Daniel Michalik, who wintered at the Amundsen–Scott South Pole Station in Antarctica in 2017. It was taken as a single long exposure with minor contrast and exposure adjustments. At extremely cold temperatures of -60°C, Daniel was required to layer up, use a hot water bottle to keep the camera warm, and to pack his pockets with plentiful spare batteries. The photographer’s stoicism paid off, as the image was shortlisted as a finalist in the Royal Society photography competition in 2017. Another of Daniel’s images, published here, was the overall winner of the ‘Astronomy’ category.Between 3 and 5 March ESA is highlighting the effects of space weather with the #AuroraHunters SocialSpace event at the other ‘end’ of the planet, in Tromsø, Norway. Follow the conversation on Twitter to see more great aurora images!
Earth is not the only blue marble in the solar system, there is also Uranus (L) and Neptune (R).
Image: NASA, ESA, A. Simon (NASA Goddard Space Flight Center), and M.H. Wong and A. Hsu (University of California, Berkeley)
ESA: Sitting beyond Jupiter and Saturn in our Solar System, these two planets have only been visited once by a spacecraft, albeit briefly. NASA’s Voyager 2 spacecraft swung by Uranus in 1986, and Neptune in 1989, snapping the only close-up detailed images of these distant worlds.
The first images of Neptune revealed a planet with a dynamic atmosphere, including two mysterious dark vortices. Uranus, however, appeared featureless. But these views were just one-time snapshots: they couldn’t capture how the planets’ atmospheres change over time.
Enter the Hubble Space Telescope, which has been making a roughly annual check-up of these distant worlds as they go through protracted seasonal changes in their multi-decades-long orbits – a year on Uranus is 84 Earth years, while Neptune takes 165 of our years to orbit the Sun.
The latest pair of Hubble images are presented here, displaying Uranus (left) alive with activity and Neptune (right) showing off a new dark storm.
The vast bright polar cap across the north pole dominates the image of Uranus. The cap, which may form due to seasonal changes in atmospheric flow, has become much more prominent than in previous observations dating back to the Voyager 2 flyby, when the planet, in the throes of winter, looked bland.
Scientists believe this feature is a result of Uranus’ unique rotation. Unlike every other planet in the Solar System, Uranus is tipped over almost onto its side. Because of this extreme tilt, during the planet’s summer the Sun shines almost directly onto the north pole and never sets. Uranus is now approaching the middle of its 21 year-long summer season and the polar-cap region is becoming more prominent.
Near the edge of the cloud cap is a large cloud of methane ice, while a narrow cloud band encircles the planet north of the equator. It is a mystery how bands like these are confined to such narrow widths, because Uranus and Neptune have very broad westward-blowing wind jets.
The latest images show that Neptune has a new swirling dark storm spanning nearly 11 000 km across – roughly equivalent to the distance between Lisbon, Portugal and Tokyo, Japan. It is accompanied by bright white ‘companion clouds’ formed when the flow of ambient air is perturbed and diverted upward over the dark vortex, causing gases to freeze into methane ice crystals. Like Jupiter’s Great Red Spot, the dark vortices swirl in an anti-cyclonic direction and seem to dredge up material from deeper levels in the ice giant’s atmosphere.
Both Uranus and Neptune are classified as ‘ice giant’ planets, which are fundamentally different to the gas giants like Jupiter and Saturn. They have no solid surface but rather layers of hydrogen and helium surrounding a water-rich interior, itself perhaps wrapped around a rocky core. Atmospheric methane absorbs red light but allows blue-green light to be scattered back into space, giving each planet a characteristic cyan hue.
Analysing these worlds will help scientists better understand the diversity and similarities of the planets in our own Solar System as well as the thousands of exoplanets discovered in other solar systems – the vast majority of which fall into the size range of Neptune and Uranus.
Indeed, ESA’s upcoming exoplanet mission Cheops will focus on analysing stars that are known to host Earth to Uranus- and Neptune-sized planets, providing a first step-characterisation into the nature of these alien worlds.
Given a favourable alignment of Jupiter to provide gravity assists in the late 2020s-early 2030s, NASA and ESA have also been studying concepts to send a mission to the ice giants to better understand this little-understood class of planets.
These images were captured in late 2018 as part of the Outer Planet Atmospheres Legacy (OPAL) program, and first published on 7 February 2019. This caption is based on the original release.
What power! ESA provided a link to a Hi-Res version 3.65 MB, it’s worth the time even on slow connection.
ESA – On 28 January 2019, the first qualification model of the P120C solid-propellant motor, in the configuration for Vega-C, was static fired on the test stand at Europe’s Spaceport in French Guiana.During a burn time of 135 seconds, the P120C delivered a maximum thrust of 4650 kN. No anomalies were seen and the performance met expectations.
“In this interview the Director General discusses the Space19+ proposal including his plans for space programmes to be carried out by the Agency beyond 2019, covering all aspects of space activities: science and exploration, applications, access to space, operations, research and development. The Space19+ plan also puts ESA in a world-leading position in the emerging field of space safety and security.” — ESA
A final update to the snow saga from the day before yesterday, I finished with the snow clean up from the storm we had. I had a few centimeters of new snow to get rid of, so out I went. I managed to get the vehicles cleaned off and moved around and I didn’t lose anything that I know of (LOL). I waited until the heat of the day, -18 C. As long as nothing freezes today, being a remarkably steady -27 C, I should be fine. As a matter of fact the forecast for tomorrow includes rain, that should be fun. When I get back from taking a friend for a post-operative check up I will spend some time trying to get some of the snow from the roof it’s a lot of snow and the rain will absorb and add weight.